WebbThis leads to gravitational flexing or kneading in their centers, which can heat them—an effect called tidal heating. (A fuller explanation is given in the section on Io.) We will see … WebbIo’s Volcanic Activity and Atmosphere. By Ashley Gerard Davies and Audrey Helena Vorburger. Driven by tidal heating, Io’s extreme volcanism has created a young, impact crater–free surface dominated by hundreds of active volcanic centres. From these volcanoes erupt voluminous, low-viscosity, high-temperature silicate lavas.

TIDAL HEATING IN A MAGMA OCEAN WITHIN JUPITER

http://lunarorigin.com/tidal-heating/ WebbThis loss of internal heat cools Io, making it less responsive to Jupiter’s tidal pull, thus reducing the effectiveness of tidal heating. The heating cycle then begins again with heat building until there is another eruptive phase; the process eventually results in the resurfacing of Io with layer upon layer of flood basalts. ramsey whole life insurance

The Tidal Heating of Io - YouTube

http://elementsmagazine.org/ WebbTidal Heating. Io's activity is generated by heat deep inside its center. The force needed to keep Io in synchronous rotation with Jupiter creates bulges on Io just like the Moon creates the ocean tides on Earth. The constant change in size and orientation of Io causes friction that creates enough internal heat for volcanic eruptions to occur. ramsey whole life